Figure 2 from First Millimeter Detection of the Disk around a Young, Isolated, Planetary-mass Object

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First Millimeter Detection of the Disk around a Young, Isolated, Planetary-mass Object

Authors: Amelia Bayo, Viki Joergens, Yao Liu, Robert Brauer, Johan Olofsson, Javier Arancibia, Paola Pinilla, Sebastian Wolf, Jan Philipp Ruge, Thomas Henning, Antonella Natta, Katharine G. Johnston, Mickael Bonnefoy, Henrik Beuther, and Gael Chauvin

2017 The Astrophysical Journal Letters 841 L11.

Provider: AAS Journals

Caption: Figure 2.

Illustration of the four (five-point red stars) possible determinations of the dust mass of the disk of OTS44 depending on the adopted temperature, in an ﹩{M}_{* }\mbox{--}{M}_{\mathrm{disk}}﹩ diagram, along with comparisons with other substellar objects reported in the literature. In each panel, we outline with a box the corresponding value of ﹩{T}_{\mathrm{dust}}﹩ assumed for OTS44.

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